Testing scalar versus vector dark matter
Duarte Azevedo, Mateusz Duch, Bohdan Grzadkowski, Da Huang, Michal, Iglicki, Rui Santos

TL;DR
This paper compares scalar and vector dark matter models involving extended Higgs sectors, analyzing collider and detection constraints, and proposes methods to distinguish the models at future colliders.
Contribution
It introduces a detailed comparison of scalar and vector dark matter models with extended Higgs sectors, including collider and detection constraints, and suggests experimental strategies to differentiate them.
Findings
Certain parameter regions exclude one of the models based on experimental bounds.
The process $e^+e^- o Z + ext{DM}$ can effectively distinguish the models.
Collider and detection constraints significantly constrain the models' parameter space.
Abstract
We investigate and compare two simple models of dark matter (DM): a vector and a scalar DM model. Both models require the presence of two physical Higgs bosons and which come from mixed components of the standard Higgs doublet and a complex singlet . In the Vector model, the extra symmetry is spontaneously broken by the vacuum of the complex field . This leads to a massive gauge boson that is a DM candidate stabilized by the dark charge conjugation symmetry , . On the other hand, in the Scalar model the gauge group remains the standard one. The DM field is the imaginary component of and the stabilizing symmetry is also the dark charge conjugation (). In this case, in order to avoid spontaneous breaking, the symmetry is broken explicitly, but softly, in the scalar potential. The…
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